dc.creator | Paine, John | |
dc.creator | De Ritis, Riccardo | |
dc.creator | Ventura, Guido | |
dc.creator | Longo, Laura Mariana | |
dc.creator | Ravat, Dhananjay | |
dc.creator | Speranza, Fabio | |
dc.creator | Chiappini, Massimo | |
dc.date | 2016 | |
dc.date | 2021-10-12T15:23:08Z | |
dc.date.accessioned | 2023-07-15T03:34:35Z | |
dc.date.available | 2023-07-15T03:34:35Z | |
dc.identifier | http://sedici.unlp.edu.ar/handle/10915/126468 | |
dc.identifier | issn:0956-540X | |
dc.identifier | issn:1365-246X | |
dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/7466235 | |
dc.description | The Auca Mahuida volcano (2.03–0.88 Ma) located east of the Andean thrust front in the; Neuqu´en basin (Argentina) hosts an oil system of thermogenic origin and is affected by the; NW–SE striking-faults. Intrusive bodies and the underlying Jurassic sediments constitute the; reservoir rocks. Aeromagnetic data collected in the Auca Mahuida area detected multiple; dipolar magnetic anomalies, many of which have reverse polarity. Palaeomagnetic measurements; on rock samples collected in the field together with available age determinations indicate; that the reversely magnetized sources were mainly emplaced during the Matuyama reverse; polarity chron while the normal polarity sources were emplaced during the Olduvai and/or; Jaramillo subchrons. The location and geometry of the intrusive bodies is poorly known and; the customary magnetic inversion is rendered difficult because of multiple natural remanent; magnetization directions. To address these difficulties, a voxel inversion was applied to model; the vector residual magnetic intensity (VRMI) transformation of the observed total magnetic; intensity data. The modelling showed a 1.5 km deep, subcircular ring-shaped intrusion below; the summit of the volcano and a series of NW–SE elongated, fault-controlled intrusive bodies; to depths up to 3–4 km. Our results show that magnetic data and VRMI modelling help resolve; the geometry of the shallow plumbing system of volcanoes with remanently magnetized; sources, and estimate the depth and geometry of potential oil reservoirs in volcanic areas. | |
dc.description | Facultad de Ciencias Astronómicas y Geofísicas | |
dc.format | application/pdf | |
dc.format | 852-867 | |
dc.language | en | |
dc.rights | http://creativecommons.org/licenses/by-nc-sa/4.0/ | |
dc.rights | Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) | |
dc.subject | Geología | |
dc.subject | Física | |
dc.subject | Magnetic anomaly: modelling and interpretation | |
dc.subject | Inverse theory | |
dc.subject | Gas and hydrate systems | |
dc.subject | Backarc basin processes | |
dc.subject | Physics of magma and magma bodies | |
dc.subject | South America | |
dc.title | Inverse modelling of the reversely magnetized, shallow plumbing system hosting oil reservoirs of the Auca Mahuida volcano (Payeina retroarc, Neuquén Basin, Argentina) | |
dc.type | Articulo | |
dc.type | Articulo | |